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[en] It is the purpose of the present paper to discuss in more detail the evidence for large scale correlations between the high-energy photon sky (/b/>100) and the known local distribution of diffuse interstellar matter. In particular, evidence will be presented of fairly detailed correlations with not only the Gould's Belt with its bright 'spots' in Orion and Ophiucus but also with an other local system, the so-called Dolidze Belt, recently found visible in the COS-B data base by Bignami
Source
CEA, 75 - Paris (France); International Union of Pure and Applied Physics; 288 p; ISBN 2-7272-0057-9; 
; 1981; v. 1 p. 182-185; Commissariat a l'Energie Atomique; Paris, France; 17. International cosmic ray conference; Paris, France; 13 - 25 Jul 1981; Sold by Reidel, Dordrecht, Netherlands
; 1981; v. 1 p. 182-185; Commissariat a l'Energie Atomique; Paris, France; 17. International cosmic ray conference; Paris, France; 13 - 25 Jul 1981; Sold by Reidel, Dordrecht, Netherlands
No abstract available
Source
Israel Physical Society, Jerusalem; Bull. Isr. Phys. Soc; v. 26; 82 p; 1980; p. 11; Israel Physical Society 1980 annual meeting; Rehovot, Israel; 9 - 10 Apr 1980; ISSN 0374-2687; ; Published in summary form only.
; Published in summary form only.
[en] Ultra high energy (TeV) gamma rays have been observed by an international team working at the Whipple observatory in Arizona. These also correlate with some of the signals seen by NASA's big Gamma Ray Observatory (GRO) satellite launched by the Space Shuttle Atlantis last year
Journal
[en] The present assessment of the state-of-the-art in high energy gamma-ray source astronomy highlights the progress made by means of the COS-B mission. About 25 objects have been discovered with a sensitivity of 10 to the -10th ergs/sq cm per sec and an angular resolution of the order of 1 deg. It is noted, however, that angular resolution improvements of two orders of magnitude beyond those achieved by COS-B are required for further astronomical improvements. It is suggested that collimation could be introduced into the gamma-ray beam from the source. The only effective way of implementing such a scheme is through the use of a coded mask collimation technique
Journal
Advances in Space Research; ISSN 0273-1177; ; v. 3 p. 15-21
; v. 3 p. 15-21
No abstract available
Source
CEA, 75 - Paris (France); International Union of Pure and Applied Physics; 288 p; ISBN 2-7272-0057-9; ; 1981; v. 1 p. 181; Commissariat a l'Energie Atomique; Paris, France; 17. International cosmic ray conference; Paris, France; 13 - 25 Jul 1981; Sold by Reidel, Dordrecht, Netherlands; Published in abstract form only.
; 1981; v. 1 p. 181; Commissariat a l'Energie Atomique; Paris, France; 17. International cosmic ray conference; Paris, France; 13 - 25 Jul 1981; Sold by Reidel, Dordrecht, Netherlands; Published in abstract form only.
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